ALMA spectral line and imaging survey of a low and a high mass-loss rate AGB star between 335 and 362 GHz

L. Decin; A. M. S. Richards; T. Danilovich; W. Homan; J. A. Nuth

doi:10.1051/0004-6361/201732216

Home

All issues

Volume 615 (July 2018)

A&A, 615 (2018) A28

Full HTML

Open Access

This article has an erratum: [https://doi.org/10.1051/0004-6361/201732216e]

Table 3

Summary of final continuum image parameters.

Star	Width	Beam	rms	Imsize	Pixel
	(MHz)	(mas × mas, PA)	(mJy)	(arcsec)	(arcsec)
IK Tau	15.2e3	180 × 160, 27°	0.047	10	0.04
R Dor	11.6e3	150 × 140, −5°	0.047	7.6	0.03

Notes. Width is the continuum bandwidth (spread over total spectral span), beam and rms are the continuum restoring beam and image noise, and “imsize” denotes the area imaged.

Current usage metrics show cumulative count of Article Views (full-text article views including HTML views, PDF and ePub downloads, according to the available data) and Abstracts Views on Vision4Press platform.

Data correspond to usage on the plateform after 2015. The current usage metrics is available 48-96 hours after online publication and is updated daily on week days.

Initial download of the metrics may take a while.